The Gaseous Environment of Seyfert Galaxies

Carole Mundell

Research output: Chapter or section in a book/report/conference proceedingChapter in a published conference proceeding


The VLA has been used to image HI in a heterogeneous sample of nine Seyferts as part of a continuing investigation of the role of galactic host gas in the triggering and fueling of nuclear activity. Where previous single-dish observations indicated complex, poorly understood kinematics, improved angular resolution and sensitivity reveal tidal tails and intragroup gas, distinguish dwarfs from main disks and resolve non-linear gas dynamical features such as shocks in bars. Seyferts may be abnormally gas-rich, but a larger, statistically significant comparison of HI properties of normal and active galaxies is now required.
Original languageEnglish
Title of host publicationGas and Galaxy Evolution
EditorsJ. E. Hibbard, M. Rupen, J. H. van Gorkom
Place of PublicationSan Francisco, U. S. A.
PublisherAstronomical Society of the Pacific
ISBN (Print)1583810773
Publication statusPublished - Jan 2001

Publication series

NameASP Conference Proceedings


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